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Phillips, M. M.Simon, Joshua D.Morrell, NidiaBurns, Christopher R.Cox, NickFoley, Ryan J.Karakas, AmandaPatat, F.Sternberg, A.Williams, R.Gal Yam, AvishayHsiao, EricLeonard, D.Persson, SvenStritzinger, MaximilianThompson, I.Campillay, AbdoContreras, CarlosFolatelli, GastónFreedman, Wendy L.Hamuy Wackenhut, MarioRoth, MiguelShields, GregorySuntzeff, Nicholas B.Chomiuk, LauraIvans, IneseMadore, BarryPenprase, B.Perley, DanielPignata Libralato, GiulianoPreston, G.Soderberg, Alicia[On the Source of the Dust Extinction in Type Ia Supernovae and the Discovery of Anomalously Strong Na I Absorption]

Camps, PeterMisselt, KarlBianchi, SimoneLunttila, TuomasPinte, ChristopheNatale, GiovanniJuvela, MikaFischera, JoergFitzgerald, Michael P.Gordon, KarlBaes, MaartenSteinacker, Jürgen[Benchmarking the calculation of stochastic heating and emissivity of dust grains in the context of radiative transfer simulations]

Gall, C.Stritzinger, M.D.Ashall, C.Baron, E.Burns, C.R.Hoeflich, P.Hsiao, E.Y.Mazzali, P.A.Phillips, M.M.Filippenko, A.V.Anderson, J.P.Benetti, S.Brown, P.J.Campillay, A.Challis, P.Contreras, C.Elias De La Rosa, N.Folatelli, G.Foley, R.J.Fraser, M.Holmbo, S.Marion, G.H.Morrell, N.Pan, Y.-C.Pignata, G.Suntzeff, N.B.Taddia, F.Robledo, S.T.Valenti, S.[Two transitional type Ia supernovae located in the Fornax cluster member NGC 1404: SN 2007on and SN 2011iv]Two transitional type Ia supernovae located in the Fornax cluster member NGC 1404: SN 2007on and SN 2011iv

Aims. The windows of low extinction in the Milky Way (MW) plane are rare but important because they enable us to place structural constraints on the opposite side of the Galaxy, which has hither to been done rarely. Methods. We use the near-infrared (near-IR) images of the VISTA Variables in the ...


Minniti, D.Saito, R.K.Gonzalez, O.A.Alonso-García, J.Rejkuba, M.Barbá, R.Irwin, M.Kammers, R.Lucas, P.W.Majaess, D.Valenti, E.[A new near-IR window of low extinction in the Galactic plane]A new near-IR window of low extinction in the Galactic plane

We study metal depletion due to dust in the interstellar medium (ISM) to infer the properties of dust grains and characterize the metal and dust content of galaxies down to low metallicity and intermediate redshift z. We provide metal column densities and abundances of a sample of 70 damped Lyman...


De Cia, ALedoux, CMattsson, LPetitjean, PSrianand, RGavignaud, IJenkins, EB[Dust-depletion sequences in damped Lyman-alpha absorbers A unified picture from low-metallicity systems to the Galaxy]Dust-depletion sequences in damped Lyman-alpha absorbers A unified picture from low-metallicity systems to the Galaxy

Interstellar extinction toward the Galactic Center (GC) is large and significantly differential. Its reddening and dimming effects in red clump (RC) stars in the Galactic Bulge can be exploited to better constrain the extinction law toward the innermost Galaxy. By virtue of a deep and complete ca...


Alonso-García, J.Minniti, D.Catelan, M.Contreras Ramos, R.Gonzalez, O.A.Hempel, M.Lucas, P.W.Saito, R.K.Valenti, E.Zoccali, M.[Extinction ratios in the inner Galaxy as revealed by the VVV survey]Extinction ratios in the inner Galaxy as revealed by the VVV survey

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